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  2. Graviton - Wikipedia

    en.wikipedia.org/wiki/Graviton

    Alternatively, if gravitons are massive at all, the analysis of gravitational waves yielded a new upper bound on the mass of gravitons. The graviton's Compton wavelength is at least 1.6 × 10 16 m , or about 1.6 light-years , corresponding to a graviton mass of no more than 7.7 × 10 −23 eV / c 2 . [ 18 ]

  3. Pulsar timing array - Wikipedia

    en.wikipedia.org/wiki/Pulsar_timing_array

    The amplitudes can describe the history of how galaxies were formed. The bound on the amplitude of the background waves is called an upper limit. The amplitude of the GW background is less than the upper limit. Some supermassive black hole binaries may form a stable binary and only merge after many times the current age of the universe.

  4. Gravitational wave - Wikipedia

    en.wikipedia.org/wiki/Gravitational_wave

    A more sensitive class of detector uses a laser Michelson interferometer to measure gravitational-wave induced motion between separated 'free' masses. [101] This allows the masses to be separated by large distances (increasing the signal size); a further advantage is that it is sensitive to a wide range of frequencies (not just those near a ...

  5. Gravitational-wave observatory - Wikipedia

    en.wikipedia.org/wiki/Gravitational-wave_observatory

    A more sensitive detector uses laser interferometry to measure gravitational-wave induced motion between separated 'free' masses. [7] This allows the masses to be separated by large distances (increasing the signal size); a further advantage is that it is sensitive to a wide range of frequencies (not just those near a resonance as is the case ...

  6. LIGO - Wikipedia

    en.wikipedia.org/wiki/LIGO

    The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. [1]

  7. First observation of gravitational waves - Wikipedia

    en.wikipedia.org/wiki/First_observation_of...

    Although no neutrinos were detected, the lack of such observations provided a limit on neutrino emission from this type of gravitational wave event. [69] Observations by the Swift Gamma-Ray Burst Mission of nearby galaxies in the region of the detection, two days after the event, did not detect any new X-ray, optical or ultraviolet sources. [70]

  8. Shaking detected near Catalina was not actually an ... - AOL

    www.aol.com/news/4-0-earthquake-shakes-near...

    What was initially reported to be a 4.0 earthquake Friday morning off the coast of Catalina Island was, in fact, not an earthquake, the U.S. Geological Survey said.

  9. Gravimetry - Wikipedia

    en.wikipedia.org/wiki/Gravimetry

    Large-scale gravity anomalies can be detected from space, as a by-product of satellite gravity missions, e.g., GOCE. These satellite missions aim at the recovery of a detailed gravity field model of the Earth, typically presented in the form of a spherical-harmonic expansion of the Earth's gravitational potential, but alternative presentations ...